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Fig. 12.
Predicted emergent flux profiles for the rotating star models with Ω = [0.5, 0.6, 0.7, 0.8, 0.9], and different inclination angles such that v sin (i) = 200 km s−1 for all models. The upper and lower panels display the intermediate (kL = 103) and strong (kL = 105) line, respectively.
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